@article{1538-4357-483-1-L61,
  author={M. B. Bell and P. A. Feldman and M. J. Travers and M. C. McCarthy and C. A. Gottlieb and P. Thaddeus},
  title={Detection of HC11N in the Cold Dust Cloud TMC-1},
  journal={The Astrophysical Journal Letters},
  volume={483},
  number={1},
  pages={L61},
  url={http://stacks.iop.org/1538-4357/483/i=1/a=L61},
  year={1997},
  abstract={Two consecutive rotational transitions of the long cyanopolyyne HC 11 N, J = 39 → 38 and 38 → 37, have been detected in the cold dust cloud TMC-1 at the frequencies expected from recent laboratory measurements by Travers and coworkers, and at about the expected intensities. The astronomical lines have a mean radial velocity of 5.8(1) km s -1 , in good agreement with the shorter cyanopolyynes HC 7 N and HC 9 N observed in this very sharp line source [5.82(5) and 5.84(5) km s -1 , respectively]. The column density of HC 11 N is calculated to be 2.8 × 10 11 cm -2 . The abundance of the cyanopolyynes decreases smoothly with length to HC 11 N, the decrement from one to the next being about six for the longer carbon chains.}
}